▪ Abstract In this paper we review the properties of Lyman-break galaxies, namely starburst
galaxies at high redshifts, approximately in the range 2.5< z< 5, identified by the colors of …

We report on a complete sample of seven luminous early-type galaxies in the Hubble Ultra
Deep Field (UDF) with spectroscopic redshifts between 1.39 and 2.47, and to K AB< 23 …

We present the basic data for a large ground-based spectroscopic survey for z∼ 3 Lyman
break galaxies (LBGs), photometrically selected using rest-UV colors from very deep images …

We have investigated the mass-metallicity (MZ) relation using galaxies at 0.4< z< 1.0 from
the Gemini Deep Deep Survey (GDDS) and Canada-France Redshift Survey (CFRS). Deep …

We present the results of Near-Infrared Camera and Multi-Object Spectrometer (NICMOS)
imaging of a sample of 19 high-mass passively evolving galaxies with 1.2< z< 2, taken …

Cosmic variance is the uncertainty in observational estimates of the volume density of
extragalactic objects such as galaxies or quasars arising from the underlying large-scale …

We examine the cosmic star formation rate (SFR) and its dependence on galaxy stellar mass
over the redshift range 0.8< z< 2 using data from the Gemini Deep Deep Survey (GDDS) …

We have measured the kinematic profile of the early-type (E/S0) lens galaxy in the system
0047-281 (z= 0.485) with the Echelle Spectrograph and Imager (ESI) on the WM Keck II …

Abstract The Gemini Deep Deep Survey (GDDS) is an ultradeep (K< 20.6 mag, I< 24.5 mag)
redshift survey targeting galaxies in the" redshift desert" between z= 1 and z= 2. The primary …

We present the evolution of the rest-frame optical luminosity density j, the integrated rest-
frame optical color, and the stellar mass density, ρ*, for a sample of K s band–selected …